210 citations · 486 across the 4 of their papers we have counts for
8 papers
Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Bao-An Li, Bao-Jun Cai, Wen-Jie Xie +1
New observational data of neutron stars since GW170817 have helped improve our knowledge about nuclear symmetry energy especially at high densities. We have learned particularly: (…
Impact of NICER's Radius Measurement of PSR J0740+6620 on Nuclear Symmetry Energy at Suprasaturation Densities
Nai-Bo Zhang, Bao-An Li
By directly inverting several neutron star observables in the three-dimensional parameter space for the Equation of State of super-dense neutron-rich nuclear matter, we show that t…
The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
Nai-Bo Zhang, Bin Qi, Shou-Yu Wang
The constraints on tidal deformability of neutron stars are first extracted from GW170817 by LIGO and Virgo Collaborations but the relation between radius and tidal deforma…
Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
Bao-An Li, Plamen G. Krastev, De-Hua Wen +1
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the densi…
Implications of the mass M of PSR~J0740+6620 on the Equation of State of Super-Dense Neutron-Rich Nuclear Matter
Nai-Bo Zhang, Bao-An Li
We study implications of the very recently reported mass M of PSR~J0740+6620 on the Equation of State (EOS) of super-dense neutron-rich nuclear matt…
Relation between gravitational mass and baryonic mass for non-rotating and rapidly rotating neutron stars
He Gao, Shun-Ke Ai, Zhou-Jian Cao +5
With a selected sample of neutron star (NS) equation-of-states (EOSs) that are consistent with the current observations and have a range of maximum masses, we investigate the relat…